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Rev 215 SOST Segment rainclouds 2015-129T08:15:00-131T18:00:00 No targeted flybys; Highlights:

CIRS distant observation (ISS, VIMS, UVIS in ridealong) from 129T16:45-22:20 of and to understand the spatially resolved thermal inertia, “Pacman” shape, and global energy balance. Tethys large solar phase angle; Dione moderate. Tethys (above); Dione (below) ISS Plume PIE observation at 130T00:30 (06:35 duration); another plume non-PIE on day 151 (not SOST segment)

ISS outer irregular rock observation at 130T22:25 CIRS PDT Design for 10+ hours. The goal is to determine the dynamical state ( and pole position).

Helene Rev 215 SOST Segment, cont’d. Titan rainclouds Rhea Flyby of Polydeuces BEST EVER by a factor of 2

Polydeuces is a Dione Lagrangian that was discovered by Cassini. The goal of this observation is to study its morphology, size, albedo, and derive its composition to understand its origin and relationship to Dione and other moons. Observation starts at 129T22:20 (May 10, 2015), with a closest approach around 34,000 with a moderate solar phase angle.

This is just the resolution where features (craters, CIRS PDT Design etc.) may start to appear on this . Polydeuces, Cassini’s own satellite

Helene observing campaign

(Not a PIE) Rhea

On rev 216-217 (XD Segment) there is a ~34,000 ORS Hyperion flyby designed to cover regions that may have poorly imaged (Hyperion is in chaotic rotation, so the location will be a surprise). The solar phase angle is moderate throughout the observing period, which is ideal for mapping geologic features. Tethys Composition and thermal properties will also be studied.

The observations extend from 2015- CIRS PDT Design 151T09:22-19:00. ISS is prime with CIRS and UVIS in ridealong.

Hyperion Helene Rev 217 Dione MAPS flyby (516 km) Segment 166T15:30-169T15:29 MAPS flyby to understand Dione environment and dust and interactions between particles and the surface; focus is on N. pole. Does Dione have a native source? C/A 2015-167T20:11:52.44 RSS is also in ridealong: This key observation will substantially improve our knowledge of Dione’s interior structure and the rigidity of its crust ISS reg map view (above) Other key observations: CIRS map view (below)

Tarvos (outer moon): rotation period Rhea: CIRS inbound observation Polydeuces: clone of May 10 event ISS regional map of Dione (inbound lit) CIRS map of Dione (outbound dark) Outer moon observations

Saturn UVIS PIE